Issue |
A&A
Volume 577, May 2015
|
|
---|---|---|
Article Number | A131 | |
Number of page(s) | 6 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201525699 | |
Published online | 18 May 2015 |
Discovery of variable VHE γ-ray emission from the binary system 1FGL J1018.6–5856
1
Universität Hamburg, Institut für
Experimentalphysik, Luruper Chaussee
149, 22761
Hamburg,
Germany
2
Max-Planck-Institut für Kernphysik, PO Box 103980, 69029
Heidelberg,
Germany
3
Dublin Institute for Advanced Studies,
31 Fitzwilliam Place,
Dublin 2,
Ireland
4
National Academy of Sciences of the Republic of
Armenia, Marshall Baghramian
Avenue, 24, 0019
Yerevan,
Armenia
5
Yerevan Physics Institute, 2 Alikhanian Brothers St., 375036
Yerevan,
Armenia
6
Institut für Physik, Humboldt-Universität zu Berlin,
Newtonstr. 15, 12489
Berlin,
Germany
7
University of Namibia, Department of Physics,
Private Bag 13301, Windhoek, Namibia
8
GRAPPA, Anton Pannekoek Institute for Astronomy, University of
Amsterdam, Science Park
904, 1098 XH
Amsterdam, The
Netherlands
9
Department of Physics and Electrical Engineering, Linnaeus
University, 351
95
Växjö,
Sweden
10
Institut für Theoretische Physik, Lehrstuhl IV: Weltraum und
Astrophysik, Ruhr-Universität Bochum, 44780
Bochum,
Germany
11
GRAPPA, Anton Pannekoek Institute for Astronomy and Institute of
High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH
Amsterdam, The
Netherlands
12
Institut für Astro- und Teilchenphysik,
Leopold-Franzens-Universität Innsbruck, 6020
Innsbruck,
Austria
13
School of Chemistry & Physics, University of
Adelaide, 5005
Adelaide,
Australia
14
Centre for Space Research, North-West University,
2520 Potchefstroom, South
Africa
15
LUTH, Observatoire de Paris, CNRS, Université Paris
Diderot, 5 place Jules
Janssen, 92190
Meudon,
France
16
LPNHE, Université Pierre et Marie Curie Paris 6, Université Denis
Diderot Paris 7, CNRS/IN2P3, 4
place Jussieu, 75252
Paris Cedex 5,
France
17
Laboratoire Univers et Particules de Montpellier, Université
Montpellier 2, CNRS/IN2P3, CC 72,
place Eugène Bataillon, 34095
Montpellier Cedex 5,
France
18
DSM/Irfu, CEA Saclay, 91191
Gif-Sur-Yvette Cedex,
France
19
Astronomical Observatory, The University of Warsaw,
Al. Ujazdowskie 4, 00-478
Warsaw,
Poland
20
Aix-Marseille Université, CNRS/IN2P3, CPPM UMR 7346,
13288
Marseille,
France
21
Instytut Fizyki Jądrowej PAN, ul. Radzikowskiego 152, 31-342
Kraków,
Poland
22 Funded by EU FP7 Marie Curie, grant
agreement No. PIEF-GA-2012-332350,
23
School of Physics, University of the Witwatersrand,
1 Jan Smuts Avenue, Braamfontein,
2050
Johannesburg, South
Africa
24
Landessternwarte, Universität Heidelberg,
Königstuhl, 69117
Heidelberg,
Germany
25
Oskar Klein Centre, Department of Physics, Stockholm University,
Albanova University Center, 10691
Stockholm,
Sweden
26
Institut für Astronomie und Astrophysik, Universität
Tübingen, Sand 1,
72076
Tübingen,
Germany
27
Laboratoire Leprince-Ringuet, École Polytechnique,
CNRS/IN2P3, 91128
Palaiseau,
France
28
APC, AstroParticule et Cosmologie, Université Paris Diderot,
CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10 rue Alice Domon et Léonie
Duquet, 75205
Paris Cedex 13,
France
29
Univ. Grenoble Alpes, IPAG, 38000
Grenoble, France
CNRS, IPAG, 38000
Grenoble,
France
30
Department of Physics and Astronomy, The University of Leicester,
University Road, Leicester, LE1
7RH, UK
31
Nicolaus Copernicus Astronomical Center, ul. Bartycka
18, 00-716
Warsaw,
Poland
32
Institut für Physik und Astronomie, Universität
Potsdam, Karl-Liebknecht-Strasse
24/25, 14476
Potsdam,
Germany
33
Laboratoire d’Annecy-le-Vieux de Physique des Particules,
Université Savoie Mont-Blanc, CNRS/IN2P3, 74941
Annecy-le-Vieux,
France
34
DESY, 15738
Zeuthen,
Germany
35
Obserwatorium Astronomiczne, Uniwersytet Jagielloński, ul. Orla
171, 30-244
Kraków,
Poland
36
Université Bordeaux, CNRS/IN2P3, Centre d’Études Nucléaires de Bordeaux
Gradignan, 33175
Gradignan,
France
37
Universität Erlangen-Nürnberg, Physikalisches
Institut, Erwin-Rommel-Str.
1, 91058
Erlangen,
Germany
38
Centre for Astronomy, Faculty of Physics, Astronomy and
Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100
Torun,
Poland
39
Department of Physics, University of the Free State,
PO Box 339, Bloemfontein
9300, South
Africa
40
Heisenberg Fellow (DFG), ITA Universität Heidelberg, Germany
41
GRAPPA, Institute of High-Energy Physics, University of
Amsterdam, Science Park
904, 1098 XH
Amsterdam, The
Netherlands
42
Now at Institut de Ciències de l’Espai (IEEC-CSIC),
Campus UAB, Fac. de Ciències, Torre C5, parell,
2a planta, 08193
Barcelona,
Spain
Received: 20 January 2015
Accepted: 9 March 2015
Re-observations with the HESS telescope array of the very high-energy (VHE) source HESS J1018–589 A that is coincident with the Fermi-LAT γ-ray binary 1FGL J1018.6–5856 have resulted in a source detection significance of more than 9σ and the detection of variability (χ2/ν of 238.3/155) in the emitted γ-ray flux. This variability confirms the association of HESS J1018–589 A with the high-energy γ-ray binary detected by Fermi-LAT and also confirms the point-like source as a new VHE binary system. The spectrum of HESS J1018–589 A is best fit with a power-law function with photon index Γ = 2.20 ± 0.14stat ± 0.2sys. Emission is detected up to ~20 TeV. The mean differential flux level is (2.9 ± 0.4) × 10-13 TeV-1 cm-2 s-1 at 1 TeV, equivalent to ~1% of the flux from the Crab Nebula at the same energy. Variability is clearly detected in the night-by-night light curve. When folded on the orbital period of 16.58 days, the rebinned light curve peaks in phase with the observed X-ray and high-energy phaseograms. The fit of the HESS phaseogram to a constant flux provides evidence of periodicity at the level of Nσ> 3σ. The shape of the VHE phaseogram and measured spectrum suggest a low-inclination, low-eccentricity system with amodest impact from VHE γ-ray absorption due to pair production (τ ≲ 1 at 300 GeV).
Key words: gamma rays: stars / stars: individual: 1FGL J1018.6-5856 / radiation mechanisms: non-thermal / acceleration of particles / X-rays: binaries
© ESO, 2015
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